M. Hernanz, S. Brandt, M. Feroci, P. Orleanski, A. Santangelo, S. Schanne, Xin Wu, J. in't Zand, S. N. Zhang, Y. P. Xu, E. Bozzo, Y. Evangelista, J. L. Gálvez, … 展开作者
M. Hernanz, S. Brandt, M. Feroci, P. Orleanski, A. Santangelo, S. Schanne, Xin Wu, J. in't Zand, S. N. Zhang, Y. P. Xu, E. Bozzo, Y. Evangelista, J. L. Gálvez, C. Tenzer, F. Zwart, F. J. Lu, S. Zhang, T. X. Chen, F. Ambrosino, A. Argan, E. Del Monte, C. Budtz-Jørgensen, N. Lund, P. Olsen, C. Mansanet, R. Campana, F. Fuschino, C. Labanti, A. Rachevski, A. Vacchi, G. Zampa, N. Zampa, I. Rashevskaya, P. Bellutti, G. Borghi, F. Ficorella, A. Picciotto, N. Zorzi, O. Limousin, A. Meuris
备注：
16 pages, 15 figures, to appear in proceedings of SPIE, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS) and China National Space Administration (CNSA) currently performing an extended phase A study and proposed for a launch by 2025 in a low-earth orbit. The eXTP scientific payload envisages a suite of instruments (Spectroscopy Focusing Array, Polarimetry Focusing Array, Large Area Detector and Wide Field Monitor) offering unprecedented simultaneous wide-band X-ray timing and polarimetry sensitivity. A large European consortium is contributing to the eXTP study and it is expected to provide key hardware elements, including a Wide Field Monitor (WFM). The WFM instrument for eXTP is based on the design originally proposed for the LOFT mission within the ESA context. The eXTP/WFM envisages a wide field X-ray monitor system in the 2-50 keV energy range, achieved through the technology of the large-area Silicon Drift Detectors. The WFM will consist of 3 pairs of coded mask cameras with a total combined Field of View (FoV) of 90x180 degrees at zero response and a source localization accuracy of ~1 arcmin. In this paper we provide an overview of the WFM instrument design, including new elements with respect to the earlier LOFT configuration, and anticipated performance.
气体狭缝照相机（GSC）是国际空间站上MAXI（全天空X射线图像监视器）任务中的X射线仪器。它的设计是在2- 30千电子伏波段内每92分钟的轨道周期扫描整个天空，并在迄今为止飞行的X射线全天空监测器中达到最高的灵敏度。GSC采用大面积位置敏感正比计数器，探测器总面积为5350 cm $^2$。机载数据处理器具有格式化遥测数据以及控制正比计数器的高电压以保护它们免受粒子辐照的功能。本文介绍了仪器，机载数据处理，遥测数据格式，并从地面校准测试预期的性能规格。
Design and performance of the coded mask for the Lunar Electromagnetic Monitor in X-rays (LEM-X)
INAF, Istituto di Astrofisica e Planetologia Spaziali（意大利国家天体物理研究所，空间天体物理学与行星学研究所）；INFN, Sez. Roma Tor Vergata（意大利国家核物理研究所，罗马托维加塔分部）；University of Rome “La Sapienza”, Dept. of Physics（罗马大学，物理系）；INAF, Osservatorio Astronomico di Roma（意大利国家天体物理研究所，罗马天文台）；Agenzia Spaziale Italiana（意大利航天局）；INAF, Osservatorio di Astrofisica e Scienza dello Spazio（意大利国家天体物理研究所，天体物理学与空间科学观测站）；INFN, Sez. Bologna（意大利国家核物理研究所，博洛尼亚分部）
Simulations of a 2 x 1.5D coded aperture camera for X-ray astronomy
SRON Space Research Organization Netherlands（荷兰空间研究所）；INAF-IAPS Roma（罗马国家天体物理研究所）；Institute of Space Sciences (ICE-CSIC)（空间科学研究所）；Institut d’Estudis Espacials de Catalunya (IEEC)（加泰罗尼亚空间研究学院）
本文研究了用于X射线天文观测的2 x 1.5D编码孔径相机的设计与性能，采用IROS和MLM两种解码算法，旨在提高X射线源识别和观测精度。
Initial radiometric calibration of the High-Resolution EUV Imager ($\textrm{HRI}_\textrm{EUV}$) of the Extreme Ultraviolet Imager (EUI) instrument onboard Solar Orbiter
Royal Observatory of Belgium（比利时皇家天文台）；Institut d’Astrophysique Spatiale, CNRS, Univ. Paris-Sud, Université Paris-Saclay（空间天体物理研究所，法国国家科学研究中心，巴黎南大学，巴黎萨克雷大学）；European Commission, DG Energy, Directorate D: Nuclear Energy, Safety and ITER（欧盟委员会，能源总司，D局：核能、安全与ITER）；Laboratoire Charles Fabry, Institut d’Optique Graduate School, Université Paris-Saclay（夏尔·法布里实验室，高等光学研究院，巴黎萨克雷大学）；Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center（达沃斯物理气象观测站，世界辐射中心）；UCL-Mullard Space Science Laboratory（伦敦大学学院-穆拉德空间科学实验室）；Centre Spatial de Liège, Université de Liège（列日航天中心，列日大学）；Max Planck Institute for Solar System Research（马克斯·普朗克太阳系研究所）
Performance of the Gamma-ray Transient Monitor at the IHEP Electron-Beam Facility
Institute of High Energy Physics, Chinese Academy of Sciences（中国科学院高能物理研究所）；Guangxi University（广西大学）；Technology and Engineering Center for Space Utilization, Chinese Academy of Sciences（中国科学院空间应用工程与技术中心）
